Titlebook: Meteorological Investigations of the Upper Atmosphere; R. S. Quiroz Book 1968 American Meteorological Society 1968 Mesosphere.Ionosphere.T

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ANTH

The General Circulation of the Atmosphere Above 60 Kmons are made for tests of the present theories. Energy, momentum and mass budgets are treated. Meridional cross sections of temperature are used as the basis for the discussion of the energy budget. Meteor trail winds are used as one item in the momentum budget. Atomic oxygen and ozone are treated a

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Tidal Oscillations, Shorter Period Gravity Waves and Shear Wavescal clarification of the excitation and distribution of diurnal tidal oscillations, 2) the introduction of sequential rocketborne measurements of tidal parameters to heights of 150 km, and 3) clarification of the roles played by thermal and wind gradients, and by dissipative processes, in the propag

GORGE

Some Observations of Turbulence in the 80 to 110 Km Region of the Upper Atmospherecity probability density, the structure function, eddy diffusivities, heating rate, and the altitude and seasonal variation of the energy balance parameters of the turbulence are discussed. Some aspects of the apparent disagreement between meteor trail and chemical release measurements are presented

Synchronism

D-Region Phenomena and Stratospheric-Mesospheric Couplingon and D-region phase heights, as well as from special events and anomalies in the wintertime behavior of the lower ionosphere. The paper presents examples of annual variations of ionospheric absorption and phase height at constant solar zenith angles, the results of investigations of sunrise phenom

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AXIS

Relative Motion of Ion and Neutral Clouds technique for evaporation and the process of ionization are described. By observing the drift motions of the ionized barium clouds, the electric fields have been determined in the upper atmosphere. Results are given in particular for measurements at mid-latitudes.

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Diatribe

Meteorological Rocket Measurements in the Mesospherethe relationship between synoptic data and special mesospheric data such as isolated soundings and indirect observations of various natural phenomena (e.g., noctilucent clouds, meteor trail drifts, air glow and ionospheric inhomogeneities). Progress in upward extension of current Global Meteorologic

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from the introductory chapter in Volume 1, the intensity of the fundamental with number . (. = 1,..., 3. ? 6 or i. ? 5, etc.), characterized by normal coordinate .., may be written after Introduction of Placzeck’s simplified polarizability theory as . The occurrence of . indicates dependence on the